J1420+3439
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 5323+-78 | log g : 3.24+-0.07 | vturb : 1.51+-0.20 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| Na I | 2 | ... | -0.39+-0.10 | 2.68+-0.10 | -3.56+-0.10 | -0.38+-0.10 | 2.68+-0.10 | Na I |
| Mg I | 4 | ... | 0.33+-0.16 | 4.76+-0.16 | -2.84+-0.16 | 0.34+-0.16 | 4.76+-0.16 | Mg I |
| Ca I | 7 | ... | 0.38+-0.18 | 3.55+-0.18 | -2.79+-0.18 | 0.39+-0.18 | 3.55+-0.18 | Ca I |
| Sc II | 1 | ... | 0.42+-0.14 | 0.40+-0.14 | -2.75+-0.14 | 0.43+-0.14 | 0.40+-0.14 | Sc II |
| Ti II | 9 | ... | 0.57+-0.18 | 2.35+-0.18 | -2.60+-0.18 | 0.58+-0.18 | 2.35+-0.18 | Ti II |
| Cr I | 4 | ... | -0.71+-0.08 | 1.76+-0.08 | -3.88+-0.08 | -0.70+-0.08 | 1.76+-0.08 | Cr I |
| Fe I | 35 | ... | -0.01+-0.13 | 4.32+-0.13 | -3.18+-0.13 | -0.01+-0.13 | 4.32+-0.13 | Fe I |
| Fe II | 2 | ... | 0.30+-0.32 | 4.63+-0.32 | -2.87+-0.32 | 0.30+-0.32 | 4.63+-0.32 | Fe II |
| Ni I | 1 | ... | -0.11+-0.14 | 2.94+-0.14 | -3.28+-0.14 | -0.10+-0.14 | 2.94+-0.14 | Ni I |
| Sr II | 2 | ... | -1.33+-0.15 | -1.63+-0.15 | -4.50+-0.15 | -1.32+-0.15 | -1.63+-0.15 | Sr II |
| Ba II | 2 | ... | -0.27+-0.10 | -1.26+-0.10 | -3.44+-0.10 | -0.26+-0.10 | -1.26+-0.10 | Ba II |
| Right Ascension : 14 20 51.33 | Declination : +34 39 21.40 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| N/A | N/A | SUBARUHDS | 36000 | 17.3 | N/A | 69.5 |